Celestial hemisphere:  Northern  ·  Constellation: Aquila (Aql)  ·  Contains:  LDN 635  ·  LDN 636  ·  LDN 639  ·  NGC 6755  ·  NGC 6756  ·  PK039-02.2  ·  Sh2-74
Getting plate-solving status, please wait...
NGC 6755 and 6756, Gary Imm
Powered byPixInsight

NGC 6755 and 6756

Getting plate-solving status, please wait...
NGC 6755 and 6756, Gary Imm
Powered byPixInsight

NGC 6755 and 6756

Equipment

Loading...

Acquisition details

Loading...

Description

This image captures a pair of open clusters located 5000 light years away in the constellation of Aquila. The clusters lie in the dust clouds of the Great Rift of our galaxy. These clouds greatly dim the brightness of these clusters by at least 3 magnitudes. Also visible are some interesting dark dust lanes that flow through the image. I was tempted to crop the image to highlight the clusters, but in the end I felt that the surrounding sky was too interesting to cut out.

The full resolution view is necessary to see the clusters in detail. NGC 6755 is to the left and NGC 6756 is to the right. Some believe that this pair may be the 2nd binary open star cluster identified in the Milky Way (the first being NGC 869 and 884, the Double Cluster). A binary open cluster is two open clusters which were birthed from the same molecular cloud. But recent studies of the separation and age of these 2 clusters have determined that they likely had different origins.

NGC 6755 has 150 stars and is about 25 light years in diameter, while NGC 6756 has 40 stars and is only 5 light years in diameter. Both clusters are silhouetted against starry backgrounds but there is enough difference in magnitude with the background that the clusters are fairly easily identified. The smaller cluster is easier to spot because it is more dense.

Comments